Astrophysics and Space Science

, Volume 54, Issue 2, pp 445–452 | Cite as

The oscillation frequencies of magnetic stellar models

  • David Moss


A first-order perturbation theory method developed by Goossens to determine the perturbation to the eigenfrequencies of stellar models caused by the presence of a magnetic field is modified slightly, and applied to models with toroidal and poloidal fields. Some limitations of the analysis are pointed out.


Magnetic Field Perturbation Theory Oscillation Frequency Theory Method Stellar Model 
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Copyright information

© D. Reidel Publishing Company 1978

Authors and Affiliations

  • David Moss
    • 1
  1. 1.Dept. of MathematicsUniversity of ManchesterEngland

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